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References - Bogoliubov Laboratory of Theoretical Physics - JINR

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SPIN CONTROL BY RF FIELDS AT ACCELERATORS AND STORAGE<br />

RINGS<br />

Yu. M. Shatunov<br />

Budker Institute <strong>of</strong> Nuclear <strong>Physics</strong>, Novosibirsk, Russia<br />

Abstract<br />

The first experiments to apply RF fields for resonant beam depolarization and<br />

spin flip at the VEPP-2M storage ring were carried out more than 30 years ago [1].<br />

Later this technique was used at VEPP-2M in the experiment for comparison <strong>of</strong><br />

electron and positron anomalous magnetic moments. Recently, interest in RF spin<br />

control has appeared at proton machines. This paper describes a general approach<br />

for consideration <strong>of</strong> RF influence on spin dynamics at electron (positron) and hadron<br />

accelerators. Some practical applications <strong>of</strong> RF fields are discussed.<br />

The spin motion <strong>of</strong> a particle in electromagnetic fields is described by the BMT equation:<br />

[2]<br />

−Ω =<br />

� q0<br />

γ<br />

+ q′<br />

�<br />

dS<br />

dt = ˙ S = [Ω × S]<br />

γ B�<br />

� �<br />

q0<br />

+ + q′ [E × V] , (1)<br />

γ +1<br />

B⊥ + q0 + q ′<br />

where q0 and q ′ are normal and anomalous parts <strong>of</strong> the particle gyro-magnetic ratio;<br />

B⊥ and B� are magnetic field components along and transverse to the particle velocity<br />

V. Since in circular accelerators the one-turn energy change is relatively small, we can<br />

neglect, in the first approximation, the electric field: E =0. Following the usual approach<br />

for orbital motion, we use as the independent variable the generalized azimuth θ and<br />

subdivide the spin precession vector in two parts: Ω = W0(θ) +w(θ), where W0(θ)<br />

contains only fields on the Closed Orbit R0, while w(θ) denotes all <strong>of</strong> the other terms<br />

(contributions from closed orbit imperfection and orbital oscillations). One can treat<br />

w as a small perturbation for the spin motion.( [3]- [5]) In the accelerator vector triad<br />

ex, ey = V/V, ez =[ex × ey] components <strong>of</strong> the precession vector W0 can be presented<br />

in the linear approximation in the next form: 1<br />

W0x = ν0Kx; Kx = Bx<br />

;<br />

B0<br />

W0y = (1+a) Ky; Ky = By<br />

;<br />

B0<br />

W0z = ν0Kz; Kz = Bz<br />

, (2)<br />

where we introduce the particle magnetic anomaly a = q ′ /q0 and denote ν0 = γ · a. On<br />

the reference orbit the equation has one solution n0, which is periodic around the ring,<br />

1 We use dimensionless units: fields are normalized to mean guiding field B0 =1/2π � Bzdθ; length<br />

and time are measured correspondent in units <strong>of</strong> mean radius R and revolution time.<br />

431<br />

B0

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